Bernstein, Aaron, Naturwissenschaftliche Volksbücher, Bd. 12-16, 1897

Table of contents

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            Sonnen-Entfernung. </s>
            <s xml:id="echoid-s11610" xml:space="preserve">Iſt dieſe Entfernung in Wahrheit ge-
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            ringer, als man ſie bisher angenommen, ſo folgt daraus, daß
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            man bisher auch die Maſſe der Sonne für zu groß annahm.
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            </s>
            <s xml:id="echoid-s11611" xml:space="preserve">— Dies erkannte nun Leverrier ſofort. </s>
            <s xml:id="echoid-s11612" xml:space="preserve">— Als er daher infolge-
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            deſſen die Sonnen-Entfernung um {1/30} der bisherigen Annahme
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            verminderte, klärte ſich das Rätſel auf, und es trat eine neue
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            Harmonie an die Stelle des Widerſpruches zwiſchen dem
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            Schwung des Pendels und den Einwirkungen der Erdmaſſe
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            auf die Bahnen von Mars und Venus.</s>
            <s xml:id="echoid-s11613" xml:space="preserve"/>
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            <s xml:id="echoid-s11614" xml:space="preserve">So war die Lage der Dinge im Herbſte des Jahres 1862,
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            als der Himmel ſelber zu Gunſten ſeiner treuen Forſcher durch
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            eine Gelegenheit zum Erkunden der Wahrheit intervenirte und
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            gleichzeitig ein vielverdienter Jünger der ewigen Wahrheit auf
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            den Fittigen des Lichtes eine neue Geiſtes-Eroberung in Bezug
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            auf die Erkenntnis der Sonnenferne machte.</s>
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        <div xml:id="echoid-div303" type="section" level="1" n="249">
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            <emph style="bf">VIII. Beobachtungen des Planeten Mars im</emph>
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            <emph style="bf">Jahre 1862.</emph>
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            <s xml:id="echoid-s11616" xml:space="preserve">Im Herbſt des Jahres 1862 wurde der Sternenhimmel
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            bei hereinbrechendem Abend durch den rötlichen Lichtglanz des
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            Planeten Mars verſchönt. </s>
            <s xml:id="echoid-s11617" xml:space="preserve">Den Planeten Mars in ſolcher
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            Stellung zu ſehen, in welcher er bei Sonnenuntergang im
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            Oſten aufgeht und durch die ganze Nacht am Himmel leuchtet, um
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            im Weſten unterzugehen, wenn die Sonne morgens im Oſten
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            emporſteigt, iſt keineswegs ein ſeltenes Schauſpiel, da es ſich
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            in 780 Tagen ſtets wiederholt; </s>
            <s xml:id="echoid-s11618" xml:space="preserve">der Planet ſelbſt indeſſen er-
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            ſcheint in ſolcher Stellung ſo verſchieden an Glanz und Größe,
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            daß es mit ihm doch eine beſondere Bewandtuis haben muß.</s>
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